Quasi-Stellar Diameters and Intensity Fluctuations It is shown that there are relativistic limits on the fluctuations in brightness which may be observed for a large spherical source, and also for more general sources, so that quasi-stellar objects are probably no more than light-days in size. There is thus a possibility that they may be close to our galaxy

✍ Scribed by Terrell, J.

• Book ID: 121172500
• Publisher: American Association for the Advancement of Science
• Year: 1964
• Tongue: English
• Weight: 517 KB
• Volume: 145
• Category: Article
• ISSN: 0036-8075
• DOI: 10.1126/science.145.3635.918